Overview of the AVIRIS 2000 flight season
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Engineering topics
Publications and source records attributed to Faust, J..
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This guide serves as a brief overview of the AVIRIS instrument and its role in the field of imaging spectrometry.
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AVIRIS is a calibrated Earth-looking imaging spectrometer that measures the total upwelling spectral radiance in the solar reflected spectrum for 400 to 2500 nm.
This paper presents key aspects of the implementation, operation, calibration, georectification, and validation of AVIRIS on a low-altitude platform in the Autumn of 1998.
The Airborne Visible/Infrared Imaging Spectrometer (AVIRIS) measures spectral radiance in the solar reflected spectrum from 400 to 2500 nm.
The trap or quantum efficient detector has a quantum effciency of greater than 0.98 for the region from 450 to 900nm.
To validate AVIRIS in flight, and in-flight calibration experiment was performed for an over-flight on May 9, 1995, at Ivanpah Playa, California, USA. In-situ measurements were used to constrain a radiative transfer code and predict the total upwelling spectral radiance incident at AVIRIS.
None given. From Intro: This paper describes AVIRIS (the Airborne Visible and InfraRed Imaging Spectrometer) as a remote sensing instrument that is supported, calibrated, and maintained by JPL.